A solar adaptive optics system has been improved by using a high-speed electromagnetic deformable mirror and adopting a modified sum-of-absolute-differences algorithm in wavefront sensing. Results of laboratory experiments clearly show that the use of the mirror raises the temporal performance of the system. In solar observations, wavefront compensation using solar granules as a target is realized
Abstract: Wavefront sensor-less adaptive optics is an alternative way for correcting the wavefront a...
International audienceThemis is a 90 cm solar telescope which undergoes a rejuvenation of its scient...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...
With the goal of reducing the surface wavefront error of low-cost multi-meter-diameter mirrors from ...
Abstract The first generation solar adaptive optics (AO) system, which consists of a fine tracking l...
International audienceAn adaptive optics system with a single deformable mirror is being implemented...
Adaptive optics offer the potential to reduce the high cost and long lead time associated with manuf...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
This paper reports the performance of our modified adaptive optics system for solar observations. Th...
One major disadvantage to ground based observations is the distortion of light as it enters the Eart...
The resolution of ground-based telescopes is limited by the blurring caused by Earth’s turbulent atm...
Light traveling from a star suffers from optical distortion caused by the earth’s atmosphere. Adapti...
Abstract Adaptive optics (AO), which provides diffraction limited imaging over a field-of-view (FOV)...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
Adaptive optics is a combination of technologies whose purpose is to remove the effects of atmospher...
Abstract: Wavefront sensor-less adaptive optics is an alternative way for correcting the wavefront a...
International audienceThemis is a 90 cm solar telescope which undergoes a rejuvenation of its scient...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...
With the goal of reducing the surface wavefront error of low-cost multi-meter-diameter mirrors from ...
Abstract The first generation solar adaptive optics (AO) system, which consists of a fine tracking l...
International audienceAn adaptive optics system with a single deformable mirror is being implemented...
Adaptive optics offer the potential to reduce the high cost and long lead time associated with manuf...
The National Solar Observatory at Sacramento Peak is developing adaptive optics (AO) for solar astro...
This paper reports the performance of our modified adaptive optics system for solar observations. Th...
One major disadvantage to ground based observations is the distortion of light as it enters the Eart...
The resolution of ground-based telescopes is limited by the blurring caused by Earth’s turbulent atm...
Light traveling from a star suffers from optical distortion caused by the earth’s atmosphere. Adapti...
Abstract Adaptive optics (AO), which provides diffraction limited imaging over a field-of-view (FOV)...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
Adaptive optics is a combination of technologies whose purpose is to remove the effects of atmospher...
Abstract: Wavefront sensor-less adaptive optics is an alternative way for correcting the wavefront a...
International audienceThemis is a 90 cm solar telescope which undergoes a rejuvenation of its scient...
Concepts for future large space telescopes require an active optics system to mitigate aberrations c...